Open Access

Table D.1

Excerpt of the table summarising the properties of the K2 stars studied in this work.

EPIC G (mag) GBP - GRP (mag) MG (mag) Prot (day) Flag Sph a (ppm) log R′IRT ρ̄
201094776 15.3 0.85 5.60 11.15 ± 3.00 1 1831 –0.50
201097220 13.6 0.82 4.59 6.08 ± 1.05 0 4043 ± 85 0.25
201098208 14.8 1.29 6.59 13.04 ± 2.35 0 5827 0.20
201102172 16.2 2.43 10.05 3.45 ± –1.00 1 7464 ± 932 0.42
201103864 13.4 1.06 5.89 21.74 ± 4.99 1 4658 0.21
201114114 14.6 1.20 6.47 16.42 ± 4.29 0 1168 0.04
201116316 12.9 1.14 5.63 2.57 ± 0.45 1 15747 ± 7197 0.87
201121691 12.7 1.12 5.34 3.92 ±–1.00 1 8178 ± 2876 0.82
201123647 14.0 1.11 5.72 6.77 ± 1.10 0 15041 ± 2389 0.70
201131271 13.9 1.09 2.25 ± –1.00 1 7808 ± 1771 0.78
201132458 15.0 2.24 2.54 ± 0.38 1 14898 ± 1060 0.71
201134718 13.4 1.70 7.09 1.43 ± –1.00 1 8676 ± 1884 0.94
201140864 16.0 2.40 10.15 5.11 ± 0.82 1 19791 ± 927 0.33
201149128 15.9 2.40 10.04 2.02 ±–1.00 1 18889 ± 587 0.52
201154929 14.8 2.07 8.69 23.59 ± 4.98 1 4839 0.25
201166582 15.9 1.89 8.10 1.33 ± 0.21 1 2772 ± 928 0.30
201178569 15.8 2.42 9.57 2.70 ± 0.42 1 7211 ± 1013 –0.10
201212507 14.6 1.58 7.58 11.33 ± 3.80 0 3994 0.21
201223827 15.8 1.16 6.60 1.86 ± –1.00 1 8634 ± 1354 0.18
201235266 12.5 1.22 6.44 23.20 ± 5.01 1 4031 –5.4 0.50
201249315 14.9 1.13 6.17 2.70 ± 0.40 1 8163 ± 1781 0.82
201272989 14.3 1.58 7.48 16.16 ± –1.00 1 2293 ± 1264 0.24
201273096 14.9 1.33 6.45 14.95 ± 4.16 0 1724 0.24
201288384 10.8 1.78 5.30 ± 0.82 1 19583 ± 1776 0.80
201308300 11.8 0.75 4.46 4.48 ± 0.83 1 3121 ± 720 –6.1 0.67
201346007 15.1 2.26 9.38 17.03 ± 3.27 0 8271 0.46
201366994 15.0 1.35 5.73 0.54 ± 0.08 1 11001 ± 1141 0.57
201377225 14.4 1.90 7.61 3.18 ± 0.47 1 16981 ± 2943 0.46
201378489 13.7 1.52 6.63 28.11 ± 12.10 0 2580 –0.24
201383978 17.9 2.74 2.89 ± 1.13 1 2161 ± 625 0.01

Notes. The full version is available at the CDS. The Flag column indicates whether the stars belong to the K2-Gaia cross validate sample (1) or not (0). When possible, the Bp - Rp magnitudes are corrected with the Apsis dereddening coefficients. (a)The Sph activity index being computed on light curve segments of length min(tobs, 5 × Prot), with tobs the total observing time, we do not provide an uncertainty on Sph for targets for which the light curve is shorter than 5 × Prot. When possible, the Bp - Rp magnitudes are corrected with the Apsis dereddening coefficients.

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